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Earthquake Cycle Simulations with Rate-And-State Friction and Power-Law T Viscoelasticity

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Earthquake Cycle Simulations with Rate-And-State Friction and Power-Law T Viscoelasticity Tectonophysics 733 (2018) 232–256 Contents lists available at ScienceDirect Tectonophysics journal homepage: www.elsevier.com/locate/tecto Earthquake cycle simulations with rate-and-state friction and power-law T viscoelasticity Kali L. Allisona,*, Eric M. Dunhama,b a Department of Geophysics, Stanford University, Stanford, CA, USA b Institute for Computational and Mathematical Engineering, Stanford University, Stanford, CA, USA ARTICLE INFO ABSTRACT Keywords: We simulate earthquake cycles with rate-and-state fault friction and off-fault power-law viscoelasticity for the Earthquake cycle classic 2D antiplane shear problem of a vertical, strike-slip plate boundary fault. We investigate the interaction Viscoelastic flow between fault slip and bulk viscous flow with experimentally-based flow laws for quartz-diorite and olivine for Power-law rheology the crust and mantle, respectively. Simulations using three linear geotherms (dT/dz=20, 25, and 30 K/km) Strike-slip produce different deformation styles at depth, ranging from significant interseismic fault creep to purely bulk Brittle-ductile transition viscous flow. However, they have almost identical earthquake recurrence interval, nucleation depth, and down- Rate-and-state friction Summation-by-parts operators dip coseismic slip limit. Despite these similarities, variations in the predicted surface deformation might permit discrimination of the deformation mechanism using geodetic observations. Additionally, in the 25 and 30 K/km simulations, the crust drags the mantle; the 20 K/km simulation also predicts this, except within 10 km of the fault where the reverse occurs. However, basal tractions play a minor role in the overall force balance of the lithosphere, at least for the flow laws used in our study. Therefore, the depth-integrated stress on the fault is balanced primarily by shear stress on vertical, fault-parallel planes. Because strain rates are higher directly below the fault than far from it, stresses are also higher. Thus, the upper crust far from the fault bears a sub- stantial part of the tectonic load, resulting in unrealistically high stresses. In the real Earth, this might lead to distributed plastic deformation or formation of subparallel faults. Alternatively, fault pore pressures in excess of hydrostatic and/or weakening mechanisms such as grain size reduction and thermo-mechanical coupling could lower the strength of the ductile fault root in the lower crust and, concomitantly, off-fault upper crustal stresses. 1. Introduction more nuanced understanding of deep fault structure and controls on seismogenic depth. Friction experiments at elevated temperatures re- Understanding the structure and dynamics of the continental li- vealed a transition from velocity-weakening to velocity-strengthening thosphere and the active faults it contains is of fundamental im- steady state friction with increasing temperature (e.g., Dieterich, 1978; portance. While it is well established that faults are highly localized Ruina, 1983; Tullis and Weeks, 1986; Blanpied et al., 1991; Blanpied within the cold, brittle upper crust, less is known about fault structure et al., 1995). Drawing upon available experimental friction data and in the warmer, and more ductile, lower crust and upper mantle. Classic estimates of continental geotherms, Tse and Rice (1986) demonstrated studies of lithospheric stress profiles were based upon laboratory rock that the primary features of crustal faulting (such as seismogenic depth deformation experiments, spanning both brittle and ductile behavior, and recurrence intervals) could be reproduced in models with ideally and theoretically based thermally activated creep laws (e.g., Byerlee, elastic off-fault response. In their model, the fault continues as a loca- 1978; Goetze and Evans, 1979; Brace and Kohlstedt, 1980; Sibson, lized surface below the seismogenic depth, with tectonic displacement 1982; Sibson, 1984). The onset of creep at elevated temperatures re- accommodated by aseismic sliding at depth. This established the im- duces stress within the lithosphere below the frictional strength, portance of the frictional seismic-aseismic transition. The majority of thereby preventing seismic slip. The predicted seismogenic depth of earthquake modeling studies that followed (e.g., Rice, 1993; Lapusta ∼10 to 20 km broadly matches observed depths of seismicity. In these et al., 2000; Kaneko et al., 2011) have followed Tse and Rice (1986) by classic studies, faults below the seismogenic depth are assumed to neglecting the viscoelastic response of the off-fault material. However, broaden rapidly into wide mylonite zones (e.g., Scholz, 2002). there have been a few studies that examine the role of viscoelasticity on These concepts were refined over the following decades to provide a earthquakes, and these are discussed at the end of this introduction. * Corresponding author. E-mail address: [email protected] (K.L. Allison). https://doi.org/10.1016/j.tecto.2017.10.021 Received 20 May 2017; Received in revised form 14 October 2017; Accepted 20 October 2017 Available online 02 November 2017 0040-1951/ © 2017 Elsevier B.V. All rights reserved. K.L. Allison, E.M. Dunham Tectonophysics 733 (2018) 232–256 Studies of exhumed fault zones place constraints on the structure of upper crust and the dry upper mantle, both of which are stronger (e.g., faults, degree of localization, and deformation mechanisms at depth. Chen and Molnar, 1983; Burov and Diament, 1995). In the “crème Exhumed rocks preserve evidence of distributed ductile deformation at brûlée” model, the upper and lower crust overlie a much weaker upper depth in the form of broad mylonite zones. Some zones are relatively mantle (e.g., Jackson, 2002; Burov and Watts, 2006). The “crème narrow, such as the 1–2 km wide mylonite zone from the middle and brûlée” model is supported, in regions such as the Mojave Desert, by lower crust beneath the Alpine Fault (Norris and Cooper, 2003). Others, estimates of rheological structure from transient postseismic deforma- such as the Great Slave Lake shear zone in Canada (Hanmer, 1988), are tion and exhumed xenoliths (summarized in Fig. 3 and discussed in tens of kilometers in width. However, it is possible that this large width more detail below) (e.g., Johnson et al., 2007; Thatcher and Pollitz, characterizes a broad zone of anastomosing faults, rather than a single 2008). Less clear support includes evidence that earthquakes are con- fault (Norris and Cooper, 2003). The dynamics of shear zones at the fined to the upper and lower crust (Maggi et al., 2000), suggesting that base of the seismogenic layer is also complicated. Exhumed rocks show the upper mantle is too weak to support earthquakes, though there is mutual overprinting of mylonites and pseudotachylytes (e.g., Cole evidence that in some regions earthquakes are able to occur in the et al., 2007; Frost et al., 2011; Kirkpatrick and Rowe, 2013), which upper mantle (e.g., Inbal et al., 2016). Additionally, evidence based on argues that the same material can respond in different ways to loading measurements of the effective elastic thickness Te, which is a proxy for across a broad range of strain rates. This evidence also shows that the lithospheric strength (Watts et al., 2013), is conflicting. In some re- brittle-ductile transition takes place gradually over a range of depths. gions, Te is smaller than the seismogenic thickness (Maggi et al., 2000; Seismic imaging studies also place constraints on the structure of Jackson, 2002), which suggests that lithospheric strength resides in the faults and degree of localization at depth. Seismic reflection and re- crust, supporting the “crème brûlée” model. Interpretations of both the fraction studies show that many continental transform faults penetrate confinement of earthquakes to the crust and Te relative to the seismo- the entire crust, persisting as localized features that cut through the genic thickness are debated, however. The apparent absence of earth- Moho (Lemiszki and Brown, 1988; Vauchez and Tommasi, 2003), in- quakes in the upper mantle may result from a strong but frictionally cluding the San Andreas (Henstock et al., 1997; Lemiszki and Brown, stable upper mantle (Jackson, 2002). Additionally, others argue that Te 1988; Zhu, 2000), the San Jacinto (Miller et al., 2014), and the Dead is larger than the seismogenic thickness in some regions (Burov and Sea transform faults (Weber et al., 2004). In contrast, the Alpine Fault Watts, 2006), which suggests that the upper mantle may be strong, and and the Marlborough Fault system, both in New Zealand's South Island, thus that the “jelly sandwich” model is correct. Burov and Watts (2006) do not appear to be highly localized at the Moho. Instead they form also find that only the “jelly sandwich” model can support mountain broad zones of deformation in the lower crust and upper mantle (Klosko ranges over millions of years. It is important to bear in mind that each et al., 1999; Molnar, 1999; Wilson et al., 2004). The width of the de- of these apparently conflicting pieces of evidence measures the strength formation zones in the upper mantle beneath these faults, as inferred of the lithosphere over a different timescale. Postseismic deformation, from seismic anisotropy studies of shear-wave splitting, is quite broad: which generally favors the “crème brûlée” model, measures the 200 km for the Alpine Fault (Duclos et al., 2005; Baldock and Stern, strength of the lithosphere on the timescale of a decade, while Te 2005), 130 km for the San Andreas Fault (Bonnin et al., 2010), and measures the strength on the scale of a million years. We focus on the 20 km for the Dead Sea Fault (Rümpker et al., 2003). The Dead Sea time scale of the postseismic and interseismic periods of the earthquake Fault has accommodated comparatively little displacement, 100 km in cycle, which range from a decade to a few hundred years, and therefore contrast with 850 km for the San Andreas, and this may account for the consider the “crème brûlée” model. Furthermore, there are likely re- relatively narrow zone exhibiting anisotropy (Baldock and Stern, 2005).
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